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General Relativistic Simulations of Stellar Core Collapse and Postbounce Evolution with Boltzmann Neutrino Transport

Matthias Liebendoerfer·O. E. Bronson Messer·Anthony Mezzacappa·W. Raphael Hix
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Abstract

We present self-consistent general relativistic simulations of stellar core collapse, bounce, and postbounce evolution for 13, 15, and 20 solar mass progenitors in spherical symmetry. Our simulations implement three-flavor Boltzmann neutrino transport and standard nuclear physics. The results are compared to our corresponding simulations with Newtonian hydrodynamics and O(v/c) Boltzmann transport.

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Matthias Liebendoerfer, O. E. Bronson Messer, Anthony Mezzacappa, W. Raphael Hix. 2001-03-01. General Relativistic Simulations of Stellar Core Collapse and Postbounce Evolution with Boltzmann Neutrino Transport. https://doi.org/10.1063/1.1419594

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